PDES: SEPARATION OF VARIABLES AND OTHER METHODS
This can be rearranged to give
r^2 R′′ 1 +2rR 1 ′− 2 R 1 =−
Ar^3
0
,
where the prime denotes differentiation with respect tor. The LHS is homogeneous and
the equation can be reduced by the substitutionr=expt, and writingR 1 (r)=S(t), to
̈S+S ̇− 2 S=−A
0
exp 3t, (21.68)
where the dots indicate differentiation with respect tot.
This is an inhomogeneous second-order ODE with constant coefficients and can be
straightforwardly solved by the methods of subsection 15.2.1 to give
S(t)=c 1 expt+c 2 exp(− 2 t)−
A
10 0
exp 3t.
Recalling thatr=exptwe find
R 1 (r)=c 1 r+c 2 r−^2 −
A
10 0
r^3.
Since we are interested in the regionr<awe must havec 2 = 0 for the solution to remain
finite. Thus inside the charge distribution the electrostatic potential has the form
u 1 (r, θ, φ)=
(
c 1 r−
A
10 0
r^3
)
P 1 (cosθ). (21.69)
Outside the charge distribution (forr≥a), however, the electrostatic potential obeys
Laplace’s equation,∇^2 u= 0, and so given the symmetry of the problem and the requirement
thatu→∞asr→∞the solution must take the form
u 2 (r, θ, φ)=
∑∞
=0
B
r+1
P(cosθ). (21.70)
We can now use the boundary conditions atr=ato fix the constants in (21.69) and
(21.70). The requirement of continuity of the potential and its radial derivative atr=a
imply that
u 1 (a, θ, φ)=u 2 (a, θ, φ),
∂u 1
∂r
(a, θ, φ)=
∂u 2
∂r
(a, θ, φ).
ClearlyB=0for= 1; carrying out the necessary differentiations and settingr=ain
(21.69) and (21.70) we obtain the simultaneous equations
c 1 a−
A
10 0
a^3 =
B 1
a^2
,
c 1 −
3 A
10 0
a^2 =−
2 B 1
a^3
,
which may be solved to givec 1 =Aa^2 /(6 0 )andB 1 =Aa^5 /(15 0 ). SinceP 1 (cosθ)=cosθ,
the electrostatic potentials inside and outside the charge distribution are given, respectively,
by
u 1 (r, θ, φ)=
A
0
(
a^2 r
6
−
r^3
10
)
cosθ, u 2 (r, θ, φ)=
Aa^5
15 0
cosθ
r^2